Galaxy clusters are the most massive gravitationally bound objects in the Universe, forming at the nodes of the cosmic web [1]}, [2]}. They are excellent tools for both astrophysical and cosmological studies (see e.g. [3]}, [4]}, [5]}). The imprint of structure formation is carried by the galaxy cluster number density and spatial distribution of galaxy clusters. Hence, the abundance of galaxy clusters with mass and redshift is a well–known cosmological probe. The mass function of galaxy clusters describes the number density of clusters above a given mass \(M\) . The sensitivity of the cluster distribution, to the underlying cosmology, is well reflected by the mass function of galaxy clusters, which is exponentially sensitive to cosmological parameters [6]}.
